Hypothesis on the Large Planetary Body on the Periphery of the Solar System
A. S. Guliyev, R. A. Guliyev
Abstract
Selected aspects of the Guliyev’s hypothesis about the existence of the large planetary body on distance of 250 - 400 AU as, a factor of comets transfer, are considered. In this hypothesis the main emphasis is on the regularities in the motion of comets coming from distant regions of the solar system. The analysis covers 1249 comets observed until 2017. It is shown that there exists a plane near which the concentration of cometary perihelion. According to the hypothesis this plane having parameters Ip = 860.2; Ωp = 2710.7 is result of the influence of giant planetary body at the distance of 250 - 400 AU. It shows that number of aphelia and distant nodes of cometary orbits within this limit (within statistical validity) significantly exceeds the expected background. On the basis of collected cometary data, we have estimated orbital elements of the hypothetical planetary body: а = 337 a.e.; e = 0.14; ω = 570; Ω = 2720.7; I = 860. Key words: comets, planet X, transfer
Language: russian
Summary
A. S. Guliyev, R. A. Guliyev
Hypothesis on the Large Planetary Body on the Periphery of the Solar System // Electronic periodical “Herald of the International Academy of Sciences. Russian Section”, 2018. Issue #1: 90—93